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Hadronic flares and associated neutrinos for Markarian 421

Published online by Cambridge University Press:  24 March 2015

Antonio Marinelli ,
Barbara Patricelli  and
Nissim Fraija
Antonio Marinelli
Affiliation:
Instituto de Física, Universidad Nacional Autónoma de México, Circuito Exterior, C.U., A. Postal 70-264, 04510 México D.F., México email: antonio.marinelli@pi.infn.it, antonio.marinelli@fisica.unam.mx
Barbara Patricelli
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Circuito Exterior, C.U., A. Postal 70-264, 04510 México D.F., México email: bpatricelli@astro.unam.mx, nifraija@astro.unam.mx
Nissim Fraija
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Circuito Exterior, C.U., A. Postal 70-264, 04510 México D.F., México email: bpatricelli@astro.unam.mx, nifraija@astro.unam.mx
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Abstract

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Markarian 421 (Mrk 421) is one of the brightest, fastest and closest BL Lac objects known. Its very high energy (VHE) spectrum has been successfully modeled with both leptonic and hadronic models and no conclusive results have been achieved yet about the origin of its VHE emission. Here we investigate the possibility that a fraction of the VHE flares of Mrk 421 are due to hadronic processes and calculate the expected associated neutrino flux. We introduce the obtained neutrino flux in a Monte Carlo simulation to see the expectation for a km3 Cherenkov neutrino telescope.

Keywords

BL Lacertae objects: generalradiation mechanisms: nonthermalneutrinos
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S313: Extragalactic jets from every angle , September 2014 , pp. 177 - 178
Copyright
Copyright © International Astronomical Union 2015 

References

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